Propagation of gravitational waves in Chern-Simons axion Einstein gravity

被引:48
|
作者
Nojiri, Shin'ichi [1 ,2 ]
Odintsov, S. D. [3 ,4 ,5 ]
Oikonomou, V. K. [6 ,7 ,8 ]
Popov, Arkady A. [9 ]
机构
[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
[2] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan
[3] ICREA, Passeig Luis Co 23, Barcelona 08010, Spain
[4] Inst Space Sci IEEC CSIC, C Can Magrans S-N, Barcelona 08193, Spain
[5] Tomsk State Pedag Univ, Tomsk 634061, Russia
[6] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki 54124, Greece
[7] Tomsk State Univ Control Syst & Radioelect TUSUR, Int Lab Theoret Cosmol, Tomsk 634050, Russia
[8] Univ Tubingen, IAAT, Theoret Astrophys, Tubingen, Germany
[9] Kazan Fed Univ, NI Lobachevsky Inst Math & Mech, Kremlevskaya St 18, Kazan 420008, Russia
基金
俄罗斯基础研究基金会;
关键词
MODULATION;
D O I
10.1103/PhysRevD.100.084009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we shall investigate the propagation of gravitational waves in a flat Friedman-Robertson-Walker background, in the context of a string motivated corrected Einstein gravity. Particularly, we shall consider a misalignment axion Einstein gravity in the presence of a string originating Chern-Simons coupling of the axion field to the Chern-Pontryagin density in four dimensions. We shall focus our study on the propagation of the gravitational waves, and we shall investigate whether there exists any difference in the propagation of the polarization states of the gravitational waves. As we demonstrate, the dispersion relations are different in the right-handed mode and the left-handed mode. Finally, we compare the propagation of the axion Chern-Simons Einstein theory with that of standard F(R) gravity.
引用
收藏
页数:14
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